Dictionary of Nomenclature of Celestial Objects

  -12 094, LCLG -12 094.05
  Note:In the format, -DD denotes the central declination of the slice,    and NNN is a running number, sorted by RA within a slice.
By means of an adaptive 'friends-of-friends' percolation algorithm, a catalogue of loose groups has been produced for each of the slices from the Las Campanas Redshift Survey LCRS.
Each group consitutes a density enhancement of 80 times the mean background number density of galaxies.
See also LCDCS, LCCG, LARCS, LCRS. Ref:=2000ApJS..130..237T byTUCKER D.L. , OEMLER A.Jr, HASHIMOTO Y., SHECTMAN S.A., KIRSHNER R.P., LIN H., LANDY S.D., SCHECHTER P.L., ALLAM S.S. Astrophys. J., Suppl. Ser., 130, 237-265 (2000) Loose groups of galaxies in the Las Campanas Redshift Survey. oTables 1: <LCLG -03 NNN> (Nos 1-288), <LCLG -06 NNN> (Nos 1-147), <LCLG -12 NNN> (Nos 1-276), <LCLG -39 NNN> (Nos 1-256), <LCLG -42 NNN> (Nos 1-265), <LCLG -45 NNN> (Nos 1-263). =E=Catalogue in electronic form as J/ApJS/130/237
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